Doubt about Frame Dragging and planetary revolution

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SUMMARY

The discussion focuses on the effects of frame dragging on a satellite placed in the Sun's orbit, specifically when it revolves in the opposite direction to the Sun's spin. It concludes that while the satellite would not fall into the Sun, it would require a higher velocity for a stable orbit due to frame dragging effects. The Kerr metric is referenced to provide the velocity formula necessary for stable orbits around rotating bodies, with specific parameters defined for the Sun's spin. Additionally, the difference in proper periods between prograde and retrograde orbits is highlighted, emphasizing its independence from gravitational constant or orbital radius.

PREREQUISITES
  • Understanding of frame dragging in general relativity
  • Familiarity with the Kerr metric and its implications
  • Knowledge of orbital mechanics and stability conditions
  • Basic concepts of black hole physics, particularly rotating black holes
NEXT STEPS
  • Study the Kerr metric in detail to understand its applications in rotating black holes
  • Explore the concept of frame dragging and its effects on satellite orbits
  • Research the differences between prograde and retrograde orbits in gravitational fields
  • Examine the implications of proper time differences in rotating systems
USEFUL FOR

Astronomers, physicists, and students of general relativity interested in the dynamics of orbits around rotating celestial bodies, particularly in the context of black holes and frame dragging effects.

SreenathSkr
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Our sun rotates in counter clockwise direction and hence frame dragging will be also in that direction. Suppose if we put a satellite in sun's orbit (almost circular) to revolve in opposite direction to the sun's spin, what would happen to the orbit of the satellite? Would it fall into the sun?
 
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Hmmm... I don't think the satellite would fall into the Sun, but I'm not certain.
 
Of course, the effect for our Sun is negligible
So it is better to talk about the rotating BH. Black holes (not rotating) have zones where no stable orbits are possible. Rotating BHs have ergosphere where you can rotate only in the same direction with BH. I think the question "what is an area where stable orbits with a rotation opposite to the BH" is a good one and is quite complicated.
 
You'll probably find that the satellite orbiting against the suns rotation would need a slightly higher velocity. From Kerr metric, the velocity required for a stable orbit at the equator around a spinning object which takes into account frame dragging is-

v_\pm=\frac{r^2+a^2\mp 2a\sqrt{Mr}}{\sqrt{\Delta} \left[a\pm r\sqrt{r/M}\right]}

where \Delta= r^{2}+a^{2}-2Mr

\pm denotes prograde and retrograde orbit, M is the gravitational radius (M=Gm/c^2) and a is the spin parameter (a=J/mc) which for the sun is approx. a=0.185M.

Source- http://arxiv.org/abs/gr-qc/0407004 equation 25
 
Very interesting, Steve... Furthermore, a prograde equatorial orbiting clock and a retrograde orbiting clock would have different proper periods, t, ...
the difference given by ...
(t+) −(t−) ≈ 4πJ/(Mc^2).
And which, remarkably, is not dependent upon G or the orbital radius...as pointed out here: http://arxiv.org/abs/gr-qc/9912027
 

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